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Post Info TOPIC: Red giants


L

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RE: Red giants
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Title: Mass-loss from Red Giants
Authors: Brian Espey, Cian Crowley

Although much is known about the nature of winds from hot stars and giants and supergiants with spectral types earlier than K, t here is still much to be learned regarding the mass-loss process in cool, late-type stars. We will review the current state of research, with particular reference to observations and modelling of mass-loss from giant stars in symbiotic systems.

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L

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When stars like our sun die, they bloat to become red giants and then eject gigantic clouds of gas and dust into space. Increasingly, however, scientists found themselves at a profound loss to explain how exactly dying stars could blow away these clouds.
Now astrophysicists propose that unexpected chemical reactions during the formation of stardust could help solve this mystery.

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